other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
1999ApJ...522..904M - Astrophys. J., 522, 904-914 (1999/September-2)
An analysis of 17 years of Voyager observations of the diffuse far-ultraviolet radiation field.
MURTHY J., HALL D., EARL M., HENRY R.C. and HOLBERG J.B.
Abstract (from CDS):
We have modeled and characterized the observed heliospheric H I and He I emission lines in the outer solar system as a function of heliospheric distance, apex angle from the direction of the inflowing interstellar wind, and time as specified by subspacecraft solar intensity. This modeling adequately reproduces observed intensities over a range of heliospheric distances of 15-50 AU, for an unrestricted range of look directions, and for a 12 year period (covering 1 solar cycle).
Abstract Copyright: ∼
Journal keyword(s): Cosmology: Diffuse Radiation - Ultraviolet: ISM
Simbad objects: 12
To bookmark this query, right click on this link: simbad:1999ApJ...522..904M and select 'bookmark this link' or equivalent in the popup menu